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A Deep Ultraviolet Raman and Fluorescence Spectral Library of 51 Organic Compounds for the SHERLOC Instrument Onboard Mars 2020.
Razzell Hollis, Joseph; Sharma, Sunanda; Abbey, William; Bhartia, Rohit; Beegle, Luther; Fries, Marc; Hein, Jeffrey D; Monacelli, Brian; Nordman, Austin D.
Afiliação
  • Razzell Hollis J; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
  • Sharma S; Department of Life Sciences, The Natural History Museum, London, United Kingdom.
  • Abbey W; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
  • Bhartia R; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
  • Beegle L; Photon Systems, Covina, California, USA.
  • Fries M; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
  • Hein JD; NASA Johnson Space Center, Houston, Texas, USA.
  • Monacelli B; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
  • Nordman AD; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
Astrobiology ; 23(1): 1-23, 2023 01.
Article em En | MEDLINE | ID: mdl-36367974
ABSTRACT
We report deep ultraviolet (DUV) Raman and Fluorescence spectra obtained on a SHERLOC (Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals) analog instrument for 51 pure organic compounds, including 5 carboxylic acids, 10 polycyclic aromatic hydrocarbons, 24 amino acids, 6 nucleobases, and 6 different grades of macromolecular carbon from humic acid to graphite. Organic mixtures were not investigated. We discuss how the DUV fluorescence and Raman spectra exhibited by different organic compounds allow for detection, classification, and identification of organics by SHERLOC. We find that 1- and 2-ring aromatic compounds produce detectable fluorescence within SHERLOC's spectral range (250-355 nm), but fluorescence spectra are not unique enough to enable easy identification of particular compounds. However, both aromatic and aliphatic compounds can be identified by their Raman spectra, with the number of Raman peaks and their positions being highly specific to chemical structure, within SHERLOC's reported spectral uncertainty of ±5 cm-1. For compounds that are not in the Library, classification is possible by comparing the general number and position of dominant Raman peaks with trends for different kinds of organic compounds.
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Texto completo: 1 Base de dados: MEDLINE Assunto principal: Marte / Grafite Idioma: En Revista: Astrobiology Assunto da revista: BIOLOGIA Ano de publicação: 2023 Tipo de documento: Article País de afiliação: Estados Unidos

Texto completo: 1 Base de dados: MEDLINE Assunto principal: Marte / Grafite Idioma: En Revista: Astrobiology Assunto da revista: BIOLOGIA Ano de publicação: 2023 Tipo de documento: Article País de afiliação: Estados Unidos